7.6 Viscoelasticity and the energy principle

Two extensions close the chapter. The first admits time into the constitutive law: real materials are not perfectly elastic but viscoelastic, their stress depending on the rate of strain as well as its magnitude. The second recasts equilibrium as a minimum: the deformed shape of a loaded body is the one that minimises its total potential energy — the variational principle underlying the finite-element method.

Viscoelastic materials

A perfectly elastic solid stores all the work done on it and returns it on unloading; a viscous fluid dissipates it. Polymers, gels, biological tissues, and many soft materials do both: they store some energy and dissipate the rest, and their response depends on how fast they are loaded. Two spring-and-dashpot models capture the limiting behaviours, the spring supplying an elastic stress ε\propto\varepsilon and the dashpot a viscous stress ε˙\propto\dot\varepsilon.

Both are usefully read in the frequency domain. Driven at angular frequency ω\omega, a viscoelastic element presents a complex mechanical impedance

Z(ω)  =  b  +  i ⁣(ωmkω),Z(\omega) \;=\; b \;+\; i\!\left(\omega m - \frac{k}{\omega}\right),
where
Z(ω)Z(\omega)
mechanical impedance (force per unit velocity) N·s/m
bb
damping — the dashpot (dissipative) N·s/m
kk
stiffness — the spring (elastic) N/m
mm
inertial mass kg
ω\omega
drive angular frequency rad/s

whose real part bb measures dissipation and whose imaginary part sets the phase between force and motion. The stiffness dominates at low frequency, the mass at high, and the two cancel at resonance, where only the damping bb limits the response — the same impedance structure that governs any driven damped oscillator.

The principle of virtual work

Everything so far has been written as a differential equation — the Navier–Cauchy equation and its boundary conditions. There is an equivalent, and for computation more powerful, variational statement. The equilibrium configuration of an elastic body is the displacement field that minimises the total potential energy

Π[u]  =  V12σijεijdV    VfiuidV    StiuidS,\Pi[\mathbf{u}] \;=\; \int_V \tfrac12\,\sigma_{ij}\varepsilon_{ij}\,dV \;-\; \int_V f_i u_i\,dV \;-\; \int_S t_i u_i\,dS,
where
Π[u]\Pi[\mathbf{u}]
total potential energy functional J
12σijεij\tfrac12\sigma_{ij}\varepsilon_{ij}
stored elastic energy density J/m³
fif_i
body force per unit volume N/m³
tit_i
surface traction Pa

taken over all kinematically admissible displacement fields — those consistent with the imposed constraints. The first term is the strain energy stored in the deformation; the last two are the work done by the applied body and surface forces. Setting the first variation δΠ=0\delta\Pi = 0 recovers the Navier–Cauchy equation as its Euler–Lagrange equation, so the two formulations are equivalent.

The variational form is the foundation of the finite-element method. Rather than solve the differential equation directly, one restricts u\mathbf{u} to a finite family of shapes — piecewise-polynomial functions on a mesh of small elements — and minimises Π\Pi over the finite set of parameters. Minimising a quadratic energy over a finite-dimensional space is a linear-algebra problem, and the solution converges to the true elastic field as the mesh is refined. Nearly every structural, mechanical, and biomechanical simulation in use rests on this principle.